A Comparative Analysis of Ground, Magnetospheric and Interplanetary Observations of Long Period Magnetic Oscillations

Continuous measurements of the geomagnetic field variations at ground stations are important to investigate several aspects of magnetospheric dynamics related to variations in the solar wind conditions which, ultimately, originate from the Sun. We present a comparative analysis of geomagnetic field measurements at several ground stations with simultaneous magnetospheric and interplanetary observations in order to understand the origin and characteristics of the observed fluctuations. The results suggest that long period geomagnetic field fluctuations can be directly driven by solar wind density fluctuations at the same frequencies via the modulation of the magnetopause current. We also discuss the possible occurrence of additional contributions related with cavity/waveguide resonances of the entire magnetosphere as well as those of resonance processes of the geomagnetic field lines.     

Pc3 pulsations during variable IMF conditions

Pc3 geomagnetic field fluctuations detected at low latitude (L’Aquila, Italy) during the passage of a high velocity solar wind stream, characterized by variable interplanetary magnetic field conditions, are analyzed. Higher frequency resonant fluctuations and lower frequency phenomena are simultaneously observed; the intermittent appearance and the variable frequency of the longer period modes can be well interpreted in terms of the variable IMF elements; moreover their polarization characteristics are consistent with an origin related to external waves propagating in antisunward direction. A comparison with simultaneous observations performed at Terra Nova Bay (Antarctica) provides additional evidence for a clear relationship between the IMF and Pc3 pulsations also at very high latitudes.     

Quantitative morphometric analysis of lakes using GIS: rectangularity R,ellipticity E,orientation O,and the rectangularity vs. ellipticity index,REi

Quantitative measures of polygon shapes and orientation are important elements of geospatial analysis. These kinds of measures are particularly valuable in the case of lakes, where shape and orientation patterns can help identifying the geomorphological agents behind lake formation and evolution. However, the lack of built-in tools in commercial geographic information system (GIS) software packages designed for this kind of analysis has meant that many researchers often must rely on tools and workarounds that are not always accurate. Here, an easy-to-use method to measure rectangularity R, ellipticity E, and orientation O is developed. In addition, a new rectangularity vs. ellipticity index, REi, is defined. Following a step-by-step process, it is shown how these measures and index can be easily calculated using a combination of GIS built-in functions. The identification of shapes and estimation of orientations performed by this method is applied to the case study of the geometric and oriented lakes of the Llanos de Moxos, in the Bolivian Amazon, where shape and orientation have been the two most important elements studied to infer possible formation mechanisms. It is shown that, thanks to these new indexes, shape and orientation patterns are unveiled, which would have been hard to identify otherwise.     

Coastal defence through low crested breakwater structures: jumping out of the frying pan into the fire?

The Adriatic coast of Punta Marina (Ravenna) is protected by 3-km long low crested breakwater structures (LCSs). Through a 3-years long multidisciplinar study, we assessed the impact of such defensive structures on environmental and biological condition. LCSs create pools where conditions are very different from the surrounding nearshore system. Mechanical disturbance by currents and waves varied greatly in intensity and frequency between seaward and landward sides of the structures. Sedimentary budget was positive at the landward side, but it was due to a gain on the seafloor and not on the emerged beach. The budget at seaward was negative. LCSs determine differences in benthic assemblages, alter the seasonal pattern of communities, and modify seasonal fluctuations of animal assemblages. Landward sheltered areas can be seen as “lagoonal island” surrounded by a “sea of marine habitat”. Differences in ecological quality status, obtained through M-AMBI, are due to the sum of these factors.     

Rhyacian (2.23–2.20 Ga) juvenile accretion in the southern São Francisco craton,Brazil: Geochemical and isotopic evidence from the Serrinha magmatic suite,Mineiro belt

The Serrinha magmatic suite (Mineiro belt) crops out in the southern edge of the São Francisco craton, comprising the Brito quartz-diorite, Brumado de Cima and Brumado de Baixo granodiorites, granophyres and felsic sub-volcanic and volcanic rocks, part of which intruded into the Nazareno greenstone belt. The suite rocks have petrographic features that are consistent with magma supercooling due to the low water content combined with volatile loss, leading to crystallization of quartz and alkaline feldspar at the rims of plagioclase phenocrysts (granophyric intergrowth). The investigated rocks are sub-alkaline, calc-alkaline and show low content in rare earth elements. The U–Pb zircon crystallization ages for the Brumado de Cima granodiorite [2227 ± 22 (23) Ma] and a coeval granophyre [2211 ± 22 (23) Ma], coupled with available single-zircon Pb evaporation ages for the Brito and Brumado de Baixo plutons, are significantly older than the “Minas orogeny” (ca. 2100–2050 Ga) of Quadrilátero Ferrífero area, eastward from the Serrinha suite. Our data establish an early Rhyacian event tectonically linked with the evolution of the Mineiro belt. The bulk Nd isotopic signature [low negative to positive ε_Nd(t) values] of the Serrinha samples are consistent with the important role of Paleoproterozoic mantle components in the magma genesis. The integrated geologic, geochemical and isotopic information suggests that Paleoproterozoic evolution of the Mineiro belt initiated in a passive continental margin basin with deposition of the Minas Supergroup at ca. 2500 Ma. This stage was succeeded by outboard rupture of the oceanic lithosphere with development and coalescence of progressively younger magmatic arcs during Rhyacian time. One of the earliest arcs formed the Serrinha suite. The tectonic collage of the Serrinha and Ritápolis (2190–2120 Ma) arcs produced the NE–SW Lenheiro shear zone, resulting in mylonitization and recrystallization of both the granitoid intrusions and host rocks. As a matter of fact juxtaposition of distinct magmatic units in age and origin took place along the Lenheiros structure in this sector of the Mineiro belt.     

The precambrian evolution of South America

Zusammenfassung Mit Hilfe von ca. 1500 radiometrischen Zeitmessungen wird eine Synthese der prÄkambrischen Entwicklung Südamerikas aufgestellt. In Abb. 1 wird versucht, die Lage der spÄtprÄkambrischen orogenen Gürtel sowie ihre Plattformen darzustellen.Der grö\te alte Kern des Kontinents umfa\t den Guyana-Schild, das Basement des Amazonas-Sedimentbeckens und den Guaporé-Kraton im Süden, einen Raum von ungefÄhr 4,5 Mio. qkm. Die meisten Gesteine wurden von dem transamazonischen orogenen Zyklus erfa\t, dessen radiometrisches Alter etwa 2000 M. J. betrÄgt. Der etwa gleichaltrige SÃo-Francisco-Kraton in Ostbrasilien umfa\t ungefÄhr 1 Mio. qkm. Kleinere Kerne, die ebenfalls die Ereignisse des transamazonischen Zyklus' widerspiegeln, wurden nahe der Atlantikküste, östlich der Mündung des Amazonasflusses (SÃo-Luis-Kraton-Gebiet) und in der Umgebung des La-Plata-Flusses (Rio de la Plata-Kraton-Gebiet) gefunden.Die Kratone sind getrennt durch metamorphe Gürtel, die zum brasilianischen orogenen Zyklus spÄtprÄkambrischen Alters gehören. Der Caririan-Gürtel und die Sergipe-Geosynklinale liegen in der Nordostecke von Brasilien, und der Ribeira-Gürtel erstreckt sich entlang der Atlantikküste im Süden. Zwei symmetrische geosynklinale Einheiten wurden im zentralen Teil des Kontinents erkannt: der Brasilia- und der Paraguay-Araguaia-Gürtel.In den brasilianischen orogenen Gürteln treten an vielen Stellen transamazonische oder sogar Ältere Serien auf, Anzeichen für aufgearbeitetes altes Basement. Dies scheint zu zeigen, da\ die Sialkruste des südamerikanischen Kontinents vor 2000 M. J. schon eine rÄumliche Ausdehnung von mehr als 10 Mio. qkm hatte.

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A general synthesis of the precambrian evolution of South America has been made with the aid of about 1500 radiometric age determinations. In Fig. 1, the position of the late precambrian orogenic belts, as well as their platforms, is tentatively outlined.The largest ancient core of the continent includes the Guyana Shield, the basement of the Amazon sedimentary basin, and the Guaporé craton, to the south, covering an area of about 4.5 million square kilometers. Most of the rocks were affected by the Trans-Amazonian orogenic cycle, whose radiometric ages are close to 2000 m. y. The SÃo Francisco craton of similar age outcrops over an area of about one million square kilometers, in eastern Brazil. Smaller ancient nucleii, also reflecting the events of the Tranz-Amazonian cycle, were found near the Atlantic coast, east of the mouth of the Amazon river (SÃo Luis cratonic area), and surrounding the La Plata river (Rio de la Plata cratonic area).The old cratonic areas are separated from each other by metamorphic belts which belong to the Brazilian orogenic cycle of late precambrian age. The Caririan belt, and the Sergipe geosyncline, occur at the northeastern corner of Brazil, and the Ribeira belt along the Atlantic coast, to the south. Two symmetrical geosynclinal units were recognized in the central part of the continent: the Brasilia and the Paraguay-Araguaia belts.Within the areas of the Brazilian orogenic belts, in many places Trans-Amazonian or even older ages occur, indicating remobilized ancient basement. This seems to demonstrate that the sialic crust of the South American continent, 2000 m. y. ago, already exhibited an areal extent of more than 10 million square kilometers.

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Résumé Une synthèse générale de l'évolution précambrienne de l'Amérique du Sud a été faite à l'aide de 1500 déterminations d'âge radiométrique. La fig. 1 présente un essai sur la répartition des zones orogéniques du Précambrien supérieur et de leurs platesformes.Le noyau ancien du continent, qui est le plus vaste, comprend le bouclier de la Guyane, le socle du bassin sédimentaire de l'Amazone et le Craton de Guaporé, au Sud, couvrant une aire d'environ 4,5 millions de Km². La plupart des roches ont été affectées par le cycle orogénique Trans-Amazonien dont l'âge radiométrique est d'environ 2000 millions. Le craton de SÃo Francisco d'âge semblable, affleure sur une étendue d'environ 1 million de Km², dans l'Est du Brésil. Des noyaux anciens plus petits, affectés également par le cycle Trans-Amazonien, ont été trouvés près de la cÔte Atlantique, à l'Est de l'embouchure de l'Amazone (région cratonique de SÃo Luis), et aux environs du fleuve la Plata (région cratonique du Rio de la Plata).Les régions cratoniques anciennes sont séparées les unes des autres par des zones métamorphiques appartenant au cycle orogénique brésilien, d'âge Précambrien supérieur. La zone caririenne et le géosynclinal de Sergipe affleurent dans l'extrémité NE du Brésil, et la zone de Ribeira, le long de la cÔte Atlantique au S. Deux unités géosynclinales symétriques ont été reconnues dans la partie centrale du continent: les zones de Brasilia et de Paraguay-Araguaia.Dans les régions occupées par les ceintures orogéniques Brésiliennes, il existe en beaucoup d'endroits des roches d'âge Trans-Amazonien et mÊme plus ancien, indices d'un socle ancien remobilisé. Ceci semble démontrer que la croûte sialique du continent Sud Américain montrait déjà, il y a environ 2000 millions d'années, une étendue de plus de 10 millions de Km².

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1500 . . 1 , , . , Guaporé , . . 4,5 . , 2000 . Sao Francisco 1 . . , , , ( Sao Luis) la Plata ( (Rio de la Plata). , . Caririan Sergipe , Paraiba . : Brasilia Paraguay-Araguaia. , . , , , - , 10 . 2000 .

     

Selected solar wind parameters at 1 AU through two solar activity cycles

In situ measurements of the solar wind largely cover more than two solar magnetic activity cycles, namely 20 and 21. This is a very appealing opportunity to study the influence of the activity cycle on the behaviour of the solar wind parameters. As a matter of fact, many authors so far have studied this topic comparing the long-term magnetic field and plasma averages. However, when the average values are evaluated on a data sample whose duration is comparable with (or even longer than) the solar rotation period we lose information about the contribution due to the fast and the slow solar wind components. Thus, discriminating in velocity plays a key role in understanding solar cycle effects on the solar wind. Based on these considerations, we performed a separate analysis for fast and slow wind, respectively. In particular, we found that: (a) fast wind carries a slightly larger momentum flux density at 1 AU, probably due to dynamic stream-stream interaction; (b) proton number density in slow wind is more cycle dependent than in fast wind and decreases remarkably across solar maximum; (c) fast wind generally carries a magnetic field intensity stronger than that carried by the slow wind; (d) we found no evidence for a positive correlation between velocity and field intensity as predicted by some theories of solar wind acceleration; (e) our results would support an approximately constant divergence of field lines associated with corotating high-velocity streams.     

Constraints from geochemistry and Sr–Nd isotopes for the origin of albitite deposits from Central Sardinia (Italy)

Major- and trace-element contents and Sr–Nd isotope ratios were determined in albitite, albitized and unaltered late-Variscan granitoid samples from the world-class Na-feldspar deposits of central Sardinia, Italy. The albite deposit of high economic grade has geological, textural, and chemical features typical of metasomatic alteration affecting the host granitoids. Albitization, locally accompanied by chloritization and epidotization, was characterized by strong leaching of Mg, Fe, K, and geochemically similar trace elements, and by a significant increase of Na. Ca, and P were moderately leached in the most metasomatized rocks. Other major (Si, Ti, Ca) and trace elements (U, Th, Y, and Zr), along with light (LREE) and middle (MREE) rare-earth elements, behaved essentially immobile at the deposit scale. The Nd-isotope ratios (0.512098 to 0.512248) do not provide information on the emplacement age of the unaltered late-Variscan granitoids. On the other hand, their Sr-isotope ratios fit an errorchron of 274±29 Ma (1σ error), in fair agreement with all published ages of Sardinian Variscan granitoids. The very low Rb content of albitized rocks precludes application of the Rb–Sr radiometric system to determine the age of albitization. The Sm–Nd system is not applicable either, because the ¹⁴³Nd/¹⁴⁴Nd ratios of albitized rocks and unaltered granitoids overlap. The overlap confirms that Sm and Nd were substantially immobile during albitization. On the other hand, the measured ⁸⁷Sr/⁸⁶Sr ratios of the albitized rocks are appreciably lower than those of the unaltered host granitoids, whereas, their initial Sr-isotope ratios are higher. This seems to suggest that a) albitization was induced by non-magmatic fluids rich in radiogenic Sr, and b) albitization occurred shortly after the granitoid emplacement. This conclusion is supported by Nd isotopes, because unaltered granitoids and albitites fit the same reference isochron at 274 Ma. The fluids acquired radiogenic Sr by circulation through the Lower Paleozoic metasedimentary basement. Specifically, it is estimated that Sr supplied by the non-carbonatic basement represents about 22 wt% of total Sr in albitite.